Search Publications

Probing the Bright End of the Rest-frame Ultraviolet Luminosity Function at z = 8-10 with Hubble Pure-parallel Imaging
DOI: 10.3847/1538-4357/ab7659 Bibcode: 2020ApJ...891..146R

Finkelstein, Steven L.; Bagley, Micaela B.; Rojas-Ruiz, Sofía +5 more

Looking for bright galaxies born in the early universe is fundamental to investigating the Epoch of Reionization, the era when the first stars and galaxies ionized the intergalactic medium. We utilize Hubble Space Telescope pure-parallel imaging to select galaxy candidates at a time 500-650 million years after the Big Bang, which corresponds to re…

2020 The Astrophysical Journal
eHST 54
Chemical Evolution in the Milky Way: Rotation-based Ages for APOGEE-Kepler Cool Dwarf Stars
DOI: 10.3847/1538-4357/ab5c24 Bibcode: 2020ApJ...888...43C

van Saders, Jennifer L.; García, Rafael A.; Claytor, Zachary R. +5 more

We use models of stellar angular momentum evolution to determine ages for ∼500 stars in the APOGEE-Kepler Cool Dwarfs sample. We focus on lower-main-sequence stars, where other age-dating tools become ineffective. Our age distributions are compared to those derived from asteroseismic and giant samples and solar analogs. We are able to recover gyro…

2020 The Astrophysical Journal
Gaia 54
CLEAR. II. Evidence for Early Formation of the Most Compact Quiescent Galaxies at High Redshift
DOI: 10.3847/1538-4357/aba004 Bibcode: 2020ApJ...898..171E

Papovich, Casey; Finkelstein, Steven L.; Cleri, Nikko J. +11 more

The origin of the correlations between mass, morphology, quenched fraction, and formation history in galaxies is difficult to define, primarily due to the uncertainties in galaxy star formation histories (SFHs). SFHs are better constrained for higher redshift galaxies, observed closer to their formation and quenching epochs. Here we use "nonparame…

2020 The Astrophysical Journal
eHST 53
Microwave Spectral Imaging of an Erupting Magnetic Flux Rope: Implications for the Standard Solar Flare Model in Three Dimensions
DOI: 10.3847/2041-8213/ab901a Bibcode: 2020ApJ...895L..50C

Reeves, Katharine K.; Chen, Bin; Yu, Sijie +1 more

We report microwave spectral imaging observations of an erupting magnetic flux rope during the early impulsive phase of the X8.2-class limb flare on 2017 September 10, obtained by the Expanded Owens Valley Solar Array. A few days prior to the eruption, when viewed against the disk, the flux rope appeared as a reverse S-shaped dark filament along t…

2020 The Astrophysical Journal
Hinode 53
Multiwavelength Variability of BL Lacertae Measured with High Time Resolution
DOI: 10.3847/1538-4357/aba693 Bibcode: 2020ApJ...900..137W

Chen, W. P.; Villata, M.; Carnerero, M. I. +54 more

In an effort to locate the sites of emission at different frequencies and physical processes causing variability in blazar jets, we have obtained high time-resolution observations of BL Lacertae over a wide wavelength range: with the Transiting Exoplanet Survey Satellite (TESS) at 6000-10000 Å with 2 minute cadence; with the Neil Gehrels Swift sat…

2020 The Astrophysical Journal
Gaia 53
An Evolutionary Study of Volatile Chemistry in Protoplanetary Disks
DOI: 10.3847/1538-4357/ab9e71 Bibcode: 2020ApJ...898...97B

Wilner, David J.; Cleeves, L. Ilsedore; Andrews, Sean M. +11 more

The volatile composition of a planet is determined by the inventory of gas and ice in the parent disk. The volatile chemistry in the disk is expected to evolve over time, though this evolution is poorly constrained observationally. We present Atacama Large Millimeter/submillimeter Array observations of C18O, C2H, and the isot…

2020 The Astrophysical Journal
Gaia 53
A Very Young Radio-loud Magnetar
DOI: 10.3847/2041-8213/ab9742 Bibcode: 2020ApJ...896L..30E

Campana, S.; Tiengo, A.; Götz, D. +20 more

The magnetar Swift J1818.0-1607 was discovered in 2020 March when Swift detected a 9 ms hard X-ray burst and a long-lived outburst. Prompt X-ray observations revealed a spin period of 1.36 s, soon confirmed by the discovery of radio pulsations. We report here on the analysis of the Swift burst and follow-up X-ray and radio observations. The burst …

2020 The Astrophysical Journal
XMM-Newton 53
High-resolution Spectroscopy of the GD-1 Stellar Stream Localizes the Perturber near the Orbital Plane of Sagittarius
DOI: 10.3847/2041-8213/ab800c Bibcode: 2020ApJ...892L..37B

Conroy, Charlie; Cargile, Phillip A.; Johnson, Benjamin D. +6 more

The 100° long thin stellar stream in the Milky Way halo, GD-1, has an ensemble of features that may be due to dynamical interactions. Using high-resolution MMT/Hectochelle spectroscopy we show that a spur of GD-1-like stars outside of the main stream are kinematically and chemically consistent with the main stream. In the spur, as in the main stre…

2020 The Astrophysical Journal
Gaia 53
SPCANet: Stellar Parameters and Chemical Abundances Network for LAMOST-II Medium Resolution Survey
DOI: 10.3847/1538-4357/ab6dea Bibcode: 2020ApJ...891...23W

Luo, A. -Li; Hou, Wen; Zhang, Shuo +6 more

The fundamental stellar atmospheric parameters (Teff and log g) and 13 chemical abundances are derived for medium-resolution spectroscopy from Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Medium Resolution Survey (MRS) data sets with a deep-learning method. The neural networks we designed, named SPCANet, precisely …

2020 The Astrophysical Journal
Gaia 52
HST Proper Motions of NGC 147 and NGC 185: Orbital Histories and Tests of a Dynamically Coherent Andromeda Satellite Plane
DOI: 10.3847/1538-4357/abaf49 Bibcode: 2020ApJ...901...43S

van der Marel, Roeland P.; Geha, Marla; Fardal, Mark A. +4 more

We present the first proper-motion (PM) measurements for the dwarf elliptical galaxies NGC 147 and NGC 185, two satellite galaxies of M31, using multiepoch Hubble Space Telescope (HST) imaging data with time baselines of ∼8 yr. For each galaxy, we take an error-weighted average of measurements from HST Advanced Camera for Surveys/WFC and Wide Fiel…

2020 The Astrophysical Journal
eHST 51